Note on Shape Moduli Stabilization, String Gas Cosmology and the Swampland Criteria
arXiv:2008.13251 · doi:10.1140/epjc/s10052-021-08843-0
Abstract
In String Gas Cosmology, the simplest shape modulus fields are naturally stabilized by taking into account the presence of string winding and momentum modes. We determine the resulting effective potential for these fields and show that it obeys the de Sitter conjecture, one of the swampland criteria for effective field theories to be consistent with superstring theory.
arXiv comment4 pages
References in corpus (12)
- On the Geometry of the String Landscape and the Swampland
- The Swampland: Introduction and Review
- A Covariant Entropy Conjecture
- Bounds on Slow Roll and the de Sitter Swampland
- Producing a Scale-Invariant Spectrum of Perturbations in a Hagedorn Phase of String Cosmology
- Tensor Modes from a Primordial Hagedorn Phase of String Cosmology
- Moduli Stabilization with the String Higgs Effect
- Stabilization of Extra Dimensions at Tree Level
- Radion Stabilization by Stringy Effects in General Relativity
- The Cosmology of Massless String Modes
- Stabilizing moduli with thermal matter and nonperturbative effects
- Supersymmetry Breaking and Dilaton Stabilization in String Gas Cosmology